(1) Spatially extended Halpha and [O III] 5007 Ang emission is seen in the 2d spectrum, consistent with z=0.085. The spectrum is blue and featureless, and well fitted by a 13,000 K blackbody. Consistent with a young Type II SN a few days after explosion.
(2) Spectrum has broad P-Cygni lines in H, the Ca NIR triplet, and numerous metal lines in the blue, as seen in Type IIP SNe a few weeks into the plateau phase.
(3) Redshift measured from narrow Halpha emission. Low S/N spectrum also shows a broad emission feature at Halpha.
(4) Not visible in acquisition image.
(5) Not visible in acquisition image to a limiting magnitude of V~20.8.
(6) Spectrum is red, and dominated by host galaxy light, but SN features are visible in the blue.
(7) Spectrum has a blue continuum with narrow H emission lines at z=0.